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Titlebook: Revealing the Most Energetic Light from Pulsars and Their Nebulae; David Carreto Fidalgo Book 2019 Springer Nature Switzerland AG 2019 Cra

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發(fā)表于 2025-3-21 17:23:59 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Revealing the Most Energetic Light from Pulsars and Their Nebulae
編輯David Carreto Fidalgo
視頻videohttp://file.papertrans.cn/830/829362/829362.mp4
概述Nominated as an outstanding Ph.D. thesis by the Complutense University of Madrid, Spain.Offers a comprehensive introduction to VHE emissions from pulsars, together with a detailed compilation of VHE o
叢書名稱Springer Theses
圖書封面Titlebook: Revealing the Most Energetic Light from Pulsars and Their Nebulae; David Carreto Fidalgo Book 2019 Springer Nature Switzerland AG 2019 Cra
描述This book reports on the extraordinary observation of TeV gamma rays from the Crab Pulsar, the most energetic light ever detected from this type of object. It presents detailed information on the painstaking analysis of the unprecedentedly large dataset from the MAGIC telescopes, and comprehensively discusses the implications of pulsed TeV gamma rays for state-of-the-art pulsar emission models. Using these results, the book subsequently explores new testing methodologies for Lorentz Invariance Violation, in terms of a wavelength-dependent speed of light. The book also covers an updated search for Very-High-Energy (VHE), >100 GeV, emissions from millisecond pulsars using the Large Area Telescope on board the Fermi satellite, as well as a study on the promising Pulsar Wind Nebula candidate PSR J0631.?.The observation of VHE gamma rays is essential to studying the non-thermal sources of radiation in our Universe. Rotating neutron stars, also known as pulsars, are an extreme source class known to emit VHE gamma rays. However, to date only two pulsars have been detected with emissions above 100 GeV, and our understanding of their emission mechanism is still lacking.?.
出版日期Book 2019
關(guān)鍵詞Crab Pulsar TeV Emission; MAGIC Telescopes; VHE Gamma Rays from Pulsars; Pulsar Wind Nebula TeV Emissio
版次1
doihttps://doi.org/10.1007/978-3-030-24194-0
isbn_softcover978-3-030-24196-4
isbn_ebook978-3-030-24194-0Series ISSN 2190-5053 Series E-ISSN 2190-5061
issn_series 2190-5053
copyrightSpringer Nature Switzerland AG 2019
The information of publication is updating

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發(fā)表于 2025-3-21 21:50:52 | 只看該作者
Pulsars and Pulsar Wind Nebulaesudden stop of the free-fall collapse leads to a rebound of the infalling matter triggering an outward shock that blows up the star envelope and powers a . supernova. If the mass of the progenitor star does not exceed .20 solar masses [.], the compact remnant core evolves into a .. Otherwise the amo
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Does PSR J0631 Power a Pulsar Wind?Nebula?ost half of the current TeV .e population [.]. To increase the population with members situated in the outer part of our galaxy, . selected and observed 6 young and energetic gamma-ray pulsars that could potentially power TeV pulsar wind nebulae [.].
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MAGIC and the Crab Pulsar: History and Motivationpulsar). However, a significant portion of this 14% was taken as technical data to evaluate the performance of the instrument as described in Sect.?., and had no immediate scientific purpose. A short summary of the scientific observational campaigns on the Crab is given in Chap.?..
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發(fā)表于 2025-3-22 23:40:59 | 只看該作者
2190-5053 from pulsars, together with a detailed compilation of VHE oThis book reports on the extraordinary observation of TeV gamma rays from the Crab Pulsar, the most energetic light ever detected from this type of object. It presents detailed information on the painstaking analysis of the unprecedentedly
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An Introduction to Very-High-Energy Astrophysicsere as illustrated by Fig.?.. While for the visible and the radio part of the spectrum the atmosphere is mostly transparent, X-rays and gamma rays are completely absorbed by it. Only at the highest energy end, above a few tens of GeV, observing the violent absorption process in the atmosphere makes
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